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Nontrivial solutions for a generalized poly-Laplacian system on finite graphs

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Abstract

We investigate the existence and multiplicity of solutions for a class of the generalized coupled system involving poly-Laplacian and the parameter λ on finite graphs. By using the Mountain pass lemma together with the cut-off technique, we obtain that system has at least a nontrivial weak solution ( u λ , v λ ) for every large parameter λ when the nonlinear term F ( x , u , v ) satisfies superlinear growth conditions only in a neighborhood of origin point (0, 0). We also obtain a concrete form for the lower bound of λ and the trend of ( u λ , v λ ) with the change of λ . Moreover, by using a revised Clark’s theorem together with cut-off technique, we obtain that system has a sequence of solutions tending to 0 for every λ > 0 when the nonlinear term F ( x , u , v ) satisfies sublinear growth conditions only in a neighborhood of origin point (0, 0).

MSC 2010: 35J50; 35J62; 35B38; 35R02

1 Introduction and main results

The existence and multiplicity of solutions for the quasilinear elliptic system with the following form

(1.1) Δ p u + h 1 ( x ) u p 2 u = λ F u ( x , u , v ) , x Ω , Δ q v + h 2 ( x ) v q 2 v = λ F v ( x , u , v ) , x Ω

have been studied extensively over the past several decades (see [14] and the references therein), where Ω R N is a domain, Δ p is the so-called p -Laplacian operator, i.e., Δ p = div ( u p 2 u ) , 1 < p , q < N , λ > 0 is a parameter, and h i ( x ) ( i = 1 , 2 ) and F are real valued functions satisfying some suitable assumptions. Specially, in [1], Boccardo and Figueiredo investigated the system (1.1) with λ = 1 and h i ( x ) = 0 , i = 1 , 2, where Ω is a bounded domain in R N . They assumed that F : Ω ¯ × R × R R is of class C 1 and satisfies

F ( x , u , v ) C ( 1 + u r + v s ) ,

where C > 0 is a constant, r p * , s q * , p * = p N N p , and q * = q N N q . Moreover, there exist constants R > 0 , θ p , and θ q with 1 p * < θ p < 1 p and 1 q * < θ q < 1 q such that

0 < F ( x , u , v ) θ p u F u ( x , u , v ) + θ q v F v ( x , u , v )

for all x Ω ¯ and u , v R , which is usually called as the Ambrosseti-Rabinowitz condition and

F u ( x , u , v ) C 1 + u p * 1 + v q * ( p * 1 ) p * , F v ( x , u , v ) C 1 + v q * 1 + u p * ( q * 1 ) q * .

Under the aforementioned conditions, they established the existence result of a nontrivial solution for system (1.1) by using the Mountain pass lemma. For more results about quasilinear elliptic problems, we refer readers to [57] and the references therein.

Corresponding to system (1.1), the following well-known p -Laplacian equation

(1.2) Δ p u + h ( x ) u p 2 u = λ f ( x , u ) , x Ω

has also attracted great attention as a result of its important applications to many fields, such as non-Newtonian fluids, reaction–diffusion problems, elastic mechanics, flow through porous media, thermal radiation, and so on. For details, one can see [8] and the references therein. Specially, one of the applications of equation (1.2) is to describe the steady-state flow behavior of fluid with flow density u in the presence of interference, where h ( x ) u p 2 u and λ f ( x , u ) represent two interference sources, respectively. After the interference source h ( x ) u p 2 u disappears, (1.2) reduces to the following p -Laplacian elliptic equation

(1.3) Δ p u = λ f ( x , u ) , x Ω ,

which associated with non-Newtonian seepage phenomena [9]. At present, there are many achievements in the study of the existence of solutions to (1.2) and (1.3) (see [1013] and the references therein). In most of these articles, nonlinear term is required to have growth both near 0 and the infinity about u . In [13], Costa and Wang make some assumptions on the nonlinear term referred only to its behavior in a vicinity of u = 0 . By the cut-off technique and some estimates for solutions as the form u c 1 λ c 2 with c i > 0 ( i = 1 , 2 ) , they obtained the number of signed and sign-changing solutions for the elliptic problems (1.3) with p = 2 and f ( x , u ) = f ( u ) under the Dirichlet boundary condition u ( x ) = 0 , x Ω , where Ω R N is bounded domain. The idea in [13] has been applied to a lot of different problems, for example, Schrödinger equation [14,15] quasilinear elliptic problems involving p -Laplacian operator in R N [16] and fractional-order Kirchhoff-type system [17]. Especially, in [17], Kang et al. applied the idea to the fractional order Kirchhoff-type system with local superlinear nonlinearity. By using the Mountain pass lemma, they established the existence result of a nontrivial weak solution for every given sufficiently large λ . More importantly, they obtained a concrete value of the lower bound of the parameter λ and two estimates of weak solutions.

Recently, the subjects about the partial differential equations on graphs have attracted considerable attentions because of their applications to many fields including data analysis, image processing, neural network, transportation, and so on (see [1823] and the references therein), and there have been some works, for instance, the existence and nonexistence of solutions of heat equations [2426], the blow-up and uniqueness properties for solutions of heat equations [27,28], and the existence of solutions of Kazdan-Warner equations [29,30]. Especially, the existence and multiplicity of solutions for the poly-Laplacian system with the following form

(1.4) £ m 1 , p 1 u + h 1 ( x ) u p 1 2 u = λ F u ( x , u , v ) , x V , £ m 2 , p 2 v + h 2 ( x ) v p 2 2 v = λ F v ( x , u , v ) , x V ,

have also been investigated extensively (see [3133] and the references therein), where G = ( V , E ) is a finite graph, £ m i , p i are the poly-Laplacian operators defined in section 2, m i 1 and p i > 1 , h i ( i = 1 , 2 ) , and F are real-valued functions satisfying some assumptions. In [31], when F satisfies the super- ( p , q ) -linear growth condition, by applying the Mountain pass lemma and the Symmetric mountain pass lemma, the authors proved that the system (1.4) has at least one nontrivial solutions and dim W nontrivial solutions, where W is the working space of system (1.4), respectively. In [32], when F satisfies the asymptotically- p -linear growth conditions at infinity, the authors obtained some sufficient conditions about the existence of a nontrivial solution for system (1.4) via the Mountain pass lemma. In [33], by using the Mountain pass lemma and Ekeland’s variational principle, the authors showed that the existence of two nontrivial solutions for system (1.4) involving concave–convex nonlinearity.

In system (1.4), if we set m 1 = m 2 , p 1 = p 2 , h 1 = h 2 , λ = 1 , and u = v , it reduces to the following elliptic equation:

(1.5) £ m , p u + h ( x ) u p 2 u = f ( x , u ) ,

there are also many articles studying problem (1.5) (see [3437] and the references therein). In [34], Grigor’yan et al. studied the existence of nontrivial solution for problem (1.5) on finite graph by variational method. They assumed that f ( x , t ) satisfies the following conditions:

(f1) There exists some q > p > 1 and M > 0 such that for all x V and t M ,

0 < q F ( x , t ) t f ( x , t ) ;

(f2) limsup t 0 f ( x , t ) t p 1 < λ m p , where λ m p is the first eigenvalue of Δ p defined as follows:

λ m p = inf u 0 V ( m u p + h u p ) d μ V u p d μ .

They proved that system (1.5) admits a nontrivial solution by the Mountain pass lemma. In [35], by the same method, they established the existence result of strictly positive solutions for nonlinear equations (1.5) with m = 1 and p = 2 . They assumed that h ( x ) satisfies some reasonable assumptions and nonlinear term f ( x , t ) satisfies the following conditions:

(h1) f ( x , 0 ) = 0 , f ( x , t ) is continuous in t , and for any fixed S > 0 , there exist a constant M S such that max t [ 0 , S ] f ( x , t ) M S for all x V ;

(h2) There exists a constant μ > 2 such that for all x V and t ( 0 , + ) ,

0 < μ F ( x , t ) = μ 0 t f ( x , s ) d s t f ( x , t ) ;

(h3) limsup t 0 + 2 F ( x , t ) t 2 < λ 1 , where λ 1 is the first eigenvalue of Δ defined as follows:

λ 1 = inf V u 2 d μ = 1 V ( u 2 + h u 2 ) d μ .

Moreover, in [36], by using the Nehari method, on a locally finite graph G = ( V , E ) , Zhang and Zhao investigated the convergence of ground state solutions for equation (1.5) with m = 1 , p = 2 , h ( x ) = ς a ( x ) + 1 , and f ( x , u ) = u α 2 u , where ς is a parameter, α 2 and a ( x ) : V [ 0 , + ) . Subsequently, in [37], Han and Shao further studied the nonlinear p -Laplacian equations (1.5) with m = 1 , p 2 and h ( x ) = ς a ( x ) + 1 on a locally finite graph. Under some conditions like (h1)-(h3) on f and appropriate assumptions on a ( x ) , by the Mountain pass lemma, they proved that the aforementioned equation has a positive solution, and then by the method of Nehari manifold, they also obtained the existence of ground state solution.

Based on the works in [13,17,31,32], the motivation of our work is to consider whether the ideas in [13] can be applied to the generalized poly-Laplacian system (1.4), which is defined on finite graphs. For the super-linear case, by means of the Mountain pass lemma, we show that system (1.4) has at least a nontrivial weak solution for all parameter λ sufficiently large. Moreover, motivated by [17], we manage to find out the specific lower bound of parameter and the tendency of solution with the change of parameter. For the sublinear case, by using a revised Clark’s theorem, we obtain that system (1.4) has a sequence of solutions tending to 0 for every λ > 0 .

Our results develop those results in [17,31,32] from the following aspects:

  1. Our assumptions are different from those in [31,32]. In [31,32], the nonlinear term F needs to have growth both near (0, 0) and infinity, but all of our assumptions on F are just near the origin. It is worthwhile to mention that the existence of infinitely many solutions is not considered in [31,32].

  2. Our results are different from those in [17]. First, we focus on the generalized poly-Laplacian system (1.4) on the finite graphs, which essentially is a discrete structure, instead of the fractional order Kirchhoff-type equation on a bounded interval [ 0 , T ] studied in [17], which is a continuous structure. Moreover, in [17], the authors only considered the case that the nonlinear term F is locally superlinear. But we consider two cases: (I) the nonlinear term F is locally superlinear; (II) The nonlinear term F is locally sublinear. Finally, because of the coupling relationship of u and v and the difference between the definitions of integrals on the graph and in Euclidean space, although there are some similarities with [17] in terms of ideas, proofs in the present article are different from those in [17]. Especially, such difference can be embodied in two ways: (i) establishment of the relationship between u , v and λ (Lemma 3.5); (ii) the proofs of ( C ) c -condition holds for functional I ε (Lemma 3.4). Interestingly, it is necessary to take into account the structure of the graph when one calculates the specific lower bound of parameter, which is different from that in the Euclidean setting (Remark 5.2).

In details, we obtain the following results.

(I) The super-linear case:

Theorem 1.1

Let G = ( V , E ) be a finite graph, m i 1 and p i > 1 , i = 1 , 2, λ is a parameter with λ > 0 , h i ( x ) C ( V , R + ) , i = 1 , 2, F : V × R × R R satisfies the following conditions:

  1. There exists a constant δ > 0 such that F ( x , t , s ) is continuously differentiable in ( t , s ) R × R with ( t , s ) δ for all x V ;

  2. There exist q i > p i and M i > 0 , i = 1 , 2 such that

    F ( x , t , s ) M 1 t q 1 + M 2 s q 2

    for all x V and ( t , s ) δ ;

  3. There exist k i ( p i , q i ) ( i = 1 , 2 ) satisfy min { k 1 , k 2 } > max { p 1 , p 2 } and M j > 0 ( j = 3 , 4 ) such that

    F t ( x , t , s ) M 3 t k 1 1 + M 4 s k 2 ( k 1 1 ) k 1 , F s ( x , t , s ) M 3 t k 1 ( k 2 1 ) k 2 + M 4 s k 2 1

    for all x V and ( t , s ) δ , where F t ( x , t , s ) = F ( x , t , s ) t and F s ( x , t , s ) = F ( x , t , s ) s ;

  4. There exist constants β i > p i , i = 1 , 2 such that

    0 < F ( x , t , s ) 1 β 1 t F t ( x , t , s ) + 1 β 2 s F s ( x , t , s )

    for all x V and ( t , s ) δ with ( t , s ) ( 0 , 0 ) .

Then there exists at least a nontrivial weak solution ( u λ , v λ ) to system (1.4)for all λ > λ * max { Λ 1 , Λ 2 , Λ 3 , Λ 4 , Λ 5 } and lim λ ( u λ , v λ ) = 0 = lim λ ( u λ , v λ ) , where θ i = min { β i , k i } , i = 1 , 2, ( u 0 , v 0 ) W m 1 , p 1 ( V ) × W m 2 , p 2 ( V ) satisfies 0 < u 0 δ 2 , 0 < v 0 δ 2 for any x V , M 5 = 1 k 1 ( M 3 + M 4 ) , M 6 = k 1 1 k 1 + 1 k 2 M 4 , h i , = min x V h i ( x ) , h i = max x V h i ( x ) , i = 1 , 2, μ = min x V μ ( x ) ,

( u λ , v λ ) = u λ m 1 , p 1 + v λ m 2 , p 2 , ( u λ , v λ ) = max x V ( u λ ( x ) , v λ ( x ) ) ,

(1.6) Λ 1 = 2 1 max { p 1 , p 2 } max { p 1 , p 2 } M 5 μ k 1 p 1 p 1 h 1 , k 1 p 1 + M 6 μ k 2 p 2 p 2 h 2 , k 2 p 2 1 ,

(1.7) Λ 2 = 2 1 max { p 1 , p 2 } max { p 1 , p 2 } M 5 μ k 1 p 1 p 1 h 1 , k 1 p 1 + M 6 μ k 2 p 2 p 2 h 2 , k 2 p 2 1 6 h 1 , 1 p 1 u 0 L p 1 ( V ) max { p 1 , p 2 } min { k 1 , k 2 } ,

(1.8) Λ 3 = 2 1 max { p 1 , p 2 } max { p 1 , p 2 } M 5 μ k 1 p 1 p 1 h 1 , k 1 p 1 + M 6 μ k 2 p 2 p 2 h 2 , k 2 p 2 1 3 h 2 , 1 p 2 v 0 L p 2 ( V ) max { p 1 , p 2 } min { k 1 , k 2 } ,

(1.9) Λ 4 = 1 p 1 max { 1 , h 1 } ( m 1 u 0 L p 1 ( V ) p 1 + u 0 L p 1 ( V ) p 1 ) + 1 p 2 max { 1 , h 2 } ( m 2 v 0 L p 2 ( V ) p 2 + v 0 L p 2 ( V ) p 2 ) M 1 u 0 L p 1 ( V ) q 1 x V μ ( x ) 1 q 1 p 1 + M 2 v 0 L p 2 ( V ) q 2 x V μ ( x ) 1 q 2 p 2 ,

(1.10) Λ 5 = max 2 2 p 1 + 1 p 1 θ 1 max { C 1 , * , C 2 , * } δ p 1 ( θ 1 p 1 ) μ h 1 , 2 2 p 1 + 1 p 1 θ 1 max { C 1 , * , C 2 , * } 1 max p 1 q 1 p 1 , p 2 q 2 p 2 , × 2 2 p 2 + 1 p 2 θ 2 max { C 1 , * , C 2 , * } δ p 2 ( θ 2 p 2 ) μ h 2 , 2 2 p 2 + 1 p 2 θ 2 max { C 1 , * , C 2 , * } 1 max p 1 q 1 p 1 , p 2 q 2 p 2 ,

(1.11) C 1 , * = ( q 1 p 1 ) x V μ ( x ) p 1 ( max { 1 , h 1 } ) q 1 q 1 q 1 M 1 p 1 1 q 1 p 1 ( m 1 u 0 L p 1 ( V ) p 1 + u 0 L p 1 ( V ) p 1 ) 1 p 1 u 0 L p 1 ( V ) p 1 q 1 q 1 p 1 ,

(1.12) C 2 , * = ( q 2 p 2 ) x V μ ( x ) p 2 ( max { 1 , h 2 } ) q 2 q 2 q 2 M 2 p 2 1 q 2 p 2 ( m 2 v 0 L p 2 ( V ) p 2 + v 0 L p 2 ( V ) p 2 ) 1 p 2 v 0 L p 2 ( V ) p 2 q 2 q 2 p 2 .

Remark 1.2

It follows from ( H 1 ) and ( H 3 ) that

  1. F ( x , 0 , 0 ) = 0 for all x V .

Then by ( H 1 ) , ( H 2 ) , and ( H 4 ) , it is easy to check the following condition:
  1. M 1 t q 1 + M 2 s q 2 F ( x , t , s ) M 5 t k 1 + M 6 s k 2

    for all x V and ( t , s ) δ , where M 5 = 1 k 1 ( M 3 + M 4 ) , M 6 = ( k 1 1 k 1 + 1 k 2 ) M 4 .

(II) The sub-linear case:

Theorem 1.3

Let G = ( V , E ) be a finite graph, m i 1 , p i > 1 , i = 1 , 2, λ is a parameter with λ > 0 , h i ( x ) C ( V , R + ) , i = 1 , 2, F : V × R × R R satisfies ( H 0 ) , ( H 4 ) , and the following conditions:

  1. There exist q i ( 1 , p i ) ( i = 1 , 2 ) satisfy min { p 1 , p 2 } > max { q 1 , q 2 } and K i > 0 ( i = 1 , 2 ) such that

    F ( x , t , s ) K 1 t q 1 + K 2 s q 2

    for all x V and ( t , s ) δ ;

  2. There exist k i ( 1 , q i ) ( i = 1 , 2 ) and K j > 0 ( j = 3 , 4 ) such that

    F t ( x , t , s ) K 3 t k 1 1 + K 4 s k 2 ( k 1 1 ) k 1 , F s ( x , t , s ) K 3 t k 1 ( k 2 1 ) k 2 + K 4 s k 2 1 ,

    for all x V and ( t , s ) δ ;

  3. F ( x , t , s ) = F ( x , t , s ) for all x V and ( t , s ) δ .

Then for every λ > 0 , system (1.4) has a sequence of weak solutions { ( u k λ , v k λ ) } with ( u k λ , v k λ ) 0 as k .

Remark 1.4

By ( R 1 ) , ( R 2 ) , and ( H 4 ) , it is easy to check that the following condition:

  1. K 1 t q 1 + K 2 s q 2 F ( x , t , s ) K 5 t k 1 + K 6 s k 2

    for all x V , ( t , s ) R 2 with ( t , s ) δ , where K 5 = 1 k 1 ( K 3 + K 4 ) , K 6 = ( k 1 1 k 1 + 1 k 2 ) K 4 .

We organize this article as follows. In Section 2, we mainly recall some knowledge for poly-Laplacian on graphs and Sobolev spaces. In Section 3, we complete the proof of Theorem 1.1. In Section 4, we complete the proof of Theorem 1.3. In Section 5, we apply Theorem 1.1 to an example and compute the value of lower bound λ * . Moreover, we also present one example to illustrate Theorem 1.3.

2 Preliminaries

In this section, we recall some notions and important properties about poly-Laplacian on graphs and Sobolev spaces and some useful lemmas. One can see details in [34,36,37].

First, we recall the basic notions of weighted graphs. Let G = ( V , E ) be a finite graph, where V denotes the vertex set and E denotes the edge set. We say that a graph G = ( V , E ) is finite if and only if V and E are both finite sets. Fix an edge weight function ω : E ( 0 , + ) satisfying ω x y = ω y x , for any edge { x , y } E . Let deg ( x ) = Σ x y ω x y be the degree of x V , where we write x y if { x , y } E . Let μ : V ( 0 , + ) be a finite measure on V .

Define C ( V ) as the set of all real functions on V . Then C ( V ) is a finitely dimensional linear space with the usual functions additions and scalar multiplications. For any φ C ( V ) , we denote

(2.1) V φ d μ = x V μ ( x ) φ ( x ) .

First, for φ 1 , φ 2 C ( V ) , the associated gradient form reads

(2.2) Γ ( φ 1 , φ 2 ) ( x ) = 1 2 μ ( x ) y x ω x y ( φ 1 ( y ) φ 1 ( x ) ) ( φ 2 ( y ) φ 2 ( x ) ) .

Sometimes we use the notation φ 1 φ 2 = Γ ( φ 1 , φ 2 ) . For any φ C ( V ) , we write Γ ( φ ) = Γ ( φ , φ ) . Then the length of its gradient is defined as follows:

(2.3) φ = Γ ( φ ) = 1 2 μ ( x ) y x ω x y ( φ ( y ) φ ( x ) ) 2 1 2 .

We have the following equality:

V ( Δ φ ) ϕ d μ = V Γ ( φ , ϕ ) d μ , ϕ C c ( V ) ,

where the general discrete graph Laplacian Δ : C ( V ) C ( V ) is defined as follows:

Δ φ ( x ) = 1 μ ( x ) y x ω x y ( φ ( y ) φ ( x ) ) .

By Lemma 2.1 in [36], we know that Δ φ is well defined. Next, the length of m -order gradient of φ C ( V ) is defined by

m φ = Δ m 2 φ , when m is even , Δ m 1 2 φ , when m is odd ,

where m 1 , Δ m 2 φ is defined as the usual absolute of Δ m 2 φ and Δ m 1 2 φ denotes (2.3) with φ replaced by Δ m 1 2 φ . For any p > 1 , the p -Laplacian operator of φ C ( V ) , denoted by Δ p φ , is defined as the following form:

V ( Δ p φ ) ϕ d μ = V φ p 2 Γ ( φ , ϕ ) d μ , ϕ C c ( V ) ,

where Γ ( φ , ϕ ) is defined as in (2.2), C c ( V ) denotes the set of all real functions with compact support, and the integration is defined by (2.1). Δ p : C ( V ) C ( V ) can also be written as follows:

(2.4) Δ p φ ( x ) = 1 2 μ ( x ) y x ( φ p 2 ( y ) + φ p 2 ( x ) ) ω x y ( φ ( y ) φ ( x ) ) .

By Lemma 2.1 in [37], we know that the definition of p -Laplacian operator in (2.4) is reasonable. Now, the generalized graph poly-Laplacian £ m , p : C ( V ) C ( V ) [34] is introduced as follows:

V ( £ m , p φ ) ϕ d μ = V m φ p 2 Γ ( Δ m 1 2 φ , Δ m 1 2 ϕ ) d μ , when m is odd , V m φ p 2 Δ m 2 φ Δ m 2 ϕ d μ , when m is even ,

where m 1 , p > 1 , φ C ( V ) , ϕ C c ( V ) . It is easy to see that £ m , 2 = ( Δ ) m and £ 1 , p = Δ p .

For any 1 q < , assume that the completion space of C c ( V ) is L q ( V ) under the norm

φ L q ( V ) = V φ q d μ 1 q .

Moreover, the completion space of C c ( V ) is W m , p ( V ) under the norm

(2.5) φ m , p = V ( m φ p + h ( x ) φ p ) d μ 1 p ,

where m 1 , p > 1 , h ( x ) > 0 for all x V . Observing that W m , p ( V ) is a finite dimensional linear space and W m , p ( V ) with norm (2.5) is a Banach space. For more details about poly-Laplacian operator and Sobolev spaces on graphs, we refer readers to [34] and the reference therein.

The following inequalities and embedding proposition involving Sobolev spaces will be used frequently in our proofs.

Remark 2.1

It is easy to obtain that

h φ L p ( V ) p φ m , p p max { 1 , h } ( m φ L p ( V ) p + φ L p ( V ) p ) ,

where h = min x V h ( x ) and h = max x V h ( x ) .

Lemma 2.2

[31] Let p > 1 . For all φ W m , p ( V ) , it holds

φ 1 μ 1 p h 1 p φ m , p ,

where μ = min x V μ ( x ) .

Lemma 2.3

[31] Let G = ( V , E ) be a finite graph. Let m be any positive integer and p > 1 . Then the embedding W m , p ( V ) L q ( V ) is continuous for all 1 q < + and

φ L q ( V ) x V μ ( x ) 1 q μ 1 p h 1 p φ m , p

for all φ W m , p ( V ) . Moreover, W m , p ( V ) is pre-compact.

Next, we give an inequality, which will be used in the proof of Theorem 1.1.

Lemma 2.4

Let λ > 0 , a > 0 , and b > 0 . Then

λ a + λ b 2 ( 1 + λ max { a , b } ) .

Proof

If 0 < λ < 1 , we have λ a + λ b 2 λ max { a , b } . If λ 1 , it is obvious that λ a + λ b 2 . Then for any λ > 0 , the conclusion holds.□

Now, we recall a special version of the Mountain pass lemma. Let X be a real Banach space, I C 1 ( X , R ) and c R . A sequence { φ n } X is said to be a ( C ) c -sequence of I in X if

I ( φ n ) c , I ( φ n ) X * ( 1 + φ n ) 0 .

I is said to satisfy the ( C ) c -condition if any ( C ) c -sequence has a convergent subsequence. To prove Theorem 1.1, we need the following Mountain pass lemma.

Lemma 2.5

[38] Let X be a real Banach space, I C 1 ( X , R ) , w X , and r > 0 be such that w > r and

inf φ = r I ( φ ) > I ( 0 ) = 0 I ( w ) .

Then there exists a ( C ) c -sequence with

c inf γ Γ max t [ 0 , 1 ] I ( γ ( t ) ) , Γ { γ C ( [ 0 , 1 ] , X ) : γ ( 0 ) = 0 , γ ( 1 ) = w } .

Next, we recall an extension of Clark’s theorem. Let X be a real Banach space and I C 1 ( X , R ) . For any sequence { φ n } X , if { I ( φ n ) } is bounded and I ( φ n ) 0 as n , then { φ n } is said to be a Palais-Smale sequence of I in X . If any Palais-Smale sequence { φ n } admits a convergent subsequence, then we call that I satisfies Palais-Smale ((PS) for short) condition. To prove Theorem 1.3, we need the following Clark’s theorem.

Lemma 2.6

[39] Let X be a real Banach space and I C 1 ( X , R ) . Suppose that I satisfies the (PS)-condition, which is even, bounded from below, and I ( 0 ) = 0 . If for any k N , there exists a k-dimensional subspace Z k of X and ρ k > 0 such that sup Z k S ρ k I < 0 , where S ρ k = { φ X φ = ρ k } , then at least one of the following conclusions holds:

  1. There exist a sequence of critical points { φ k } satisfying I ( φ k ) < 0 for all k and φ k 0 as k ;

  2. There exist a constant ζ > 0 such that for any 0 < a < ζ there exists a critical point φ such that φ = a and I ( φ ) = 0 .

Remark 2.7

[39] Lemma 2.6 implies that there exist a sequence of critical points φ k 0 such that I ( φ k ) 0 , I ( φ k ) 0 , and φ k 0 as k .

3 Proofs for the super-linear case

We define the space W W m 1 , p 1 ( V ) × W m 2 , p 2 ( V ) with the norm ( u , v ) = u m 1 , p 1 + v m 2 , p 2 , where m i 1 , p i > 1 , i = 1 , 2. Then ( W , ) is a Banach space. On W , we define the variational functional corresponding to system (1.4) by

I λ ( u , v ) = 1 p 1 V ( m 1 u p 1 + h 1 ( x ) u p 1 ) d μ + 1 p 2 V ( m 2 v p 2 + h 2 ( x ) v p 2 ) d μ λ V F ( x , u , v ) d μ .

Since conditions ( H 1 ) and ( H 2 ) imply the behavior of F just near the origin, the functional V F ( x , u , v ) d μ is not well defined in the Sobolev space W . To deal with this problem, we need to extend F to a proper function F ¯ by the cut-off technique developed by [13]. To adapt system (1.4), we make an extension to R 2 for the cut-off function in [13].

Define τ ( t , s ) C 1 ( R 2 , [ 0 , 1 ] ) as a cut-off function fulfilling t τ t ( t , s ) 0 and s τ s ( t , s ) 0 for all ( t , s ) R 2 with δ 2 < ( t , s ) δ and

τ ( t , s ) = 1 , if ( t , s ) δ 2 , 0 , if ( t , s ) > δ .

Define F ¯ : V × R × R R by

F ¯ ( x , t , s ) = τ ( t , s ) F ( x , t , s ) + ( 1 τ ( t , s ) ) ( M 5 t k 1 + M 6 s k 2 ) .

By the definition of τ ( t , s ) , we could obtain the following lemma:

Lemma 3.1

Assume that ( H 0 ) , ( H 2 ) , ( H 3 ) , and ( H 5 ) hold. Then

  1. F ¯ ( x , t , s ) is continuously differentiable in ( t , s ) R × R for all x V ;

  2. there exist M 7 > 0 and M 8 > 0 such that

    F ¯ t ( x , t , s ) M 7 t k 1 1 + M 8 s k 2 ( k 1 1 ) k 1 , F ¯ s ( x , t , s ) M 7 t k 1 ( k 2 1 ) k 2 + M 8 s k 2 1 ,

    for all x V and ( t , s ) R 2 ;

  3. 0 < F ¯ ( x , t , s ) 1 θ 1 t F ¯ t ( x , t , s ) + 1 θ 2 s F ¯ s ( x , t , s )

    for all x V and ( t , s ) R 2 \ { ( 0 , 0 ) } , where θ i = min { β i , k i } , i = 1 , 2;

  4. M 1 t q 1 + M 2 s q 2 F ¯ ( x , t , s ) M 5 t k 1 + M 6 s k 2

    for all x V and ( t , s ) δ ,

    0 F ¯ ( x , t , s ) M 5 t k 1 + M 6 s k 2

    for all x V and ( t , s ) R 2 .

Consider the modified system of (1.4) given by

(3.1) £ m 1 , p 1 u + h 1 ( x ) u p 1 2 u = λ F ¯ u ( x , u , v ) , x V , £ m 2 , p 2 v + h 2 ( x ) v p 2 2 v = λ F ¯ v ( x , u , v ) , x V .

Define the corresponding functional I ¯ λ : W R by

I ¯ λ ( u , v ) 1 p 1 V ( m 1 u p 1 + h 1 ( x ) u p 1 ) d μ + 1 p 2 V ( m 2 v p 2 + h 2 ( x ) v p 2 ) d μ λ V F ¯ ( x , u , v ) d μ

for all ( u , v ) W . By ( H 0 ) , ( H 2 ) , ( H 5 ) , and the continuous embeddings

W m 1 , p 1 ( V ) L q 1 ( V ) , W m 2 , p 2 ( V ) L q 2 ( V ) ,

standard arguments show that I ¯ λ is well defined and of class C 1 on W , and

I ¯ λ ( u , v ) , ( u ˜ , v ˜ ) = V ( £ m 1 , p 1 u u ˜ + h 1 ( x ) u p 1 2 u u ˜ ) d μ + V ( £ m 2 , p 2 v v ˜ + h 2 ( x ) v p 2 2 v v ˜ ) d μ λ V F ¯ u ( x , u , v ) u ˜ d μ λ V F ¯ v ( x , u , v ) v ˜ d μ

for all ( u , v ) , ( u ˜ , v ˜ ) W [40]. Hence,

I ¯ λ ( u , v ) , ( u , v ) = u m 1 , p 1 p 1 + v m 2 , p 2 p 2 λ V F ¯ u ( x , u , v ) u d μ λ V F ¯ v ( x , u , v ) v d μ

for all ( u , v ) W . Note that the critical points of I ¯ λ with L -norm less than or equal to δ 2 are also critical points of I λ . Then the weak solutions of system (3.1) with L -norm less than or equal to δ 2 are also weak solutions of problem (1.4).

Lemma 3.2

Assume that ( H 5 ) holds. Then for each λ > 0 , there exists two positive constants ν λ and η λ such that I ¯ λ ( u , v ) η λ for all ( u , v ) = ν λ .

Proof

For any given λ > 0 , ( u , v ) W with ( u , v ) 1 , by ( H 5 ) , Lemma 2.2, Remark 2.1 and min { k 1 , k 2 } > max { p 1 , p 2 } , we have

(3.2) I ¯ λ ( u , v ) = 1 p 1 u m 1 , p 1 p 1 + 1 p 2 v m 2 , p 2 p 2 λ V F ¯ ( x , u , v ) d μ 1 max { p 1 , p 2 } ( u m 1 , p 1 max { p 1 , p 2 } + v m 2 , p 2 max { p 1 , p 2 } ) λ M 5 u k 1 p 1 u L p 1 ( V ) p 1 λ M 6 v k 2 p 2 v L p 2 ( V ) p 2 2 1 max { p 1 , p 2 } max { p 1 , p 2 } ( u , v ) max { p 1 , p 2 } λ M 5 ( μ h 1 , ) k 1 p 1 p 1 u m 1 , p 1 k 1 p 1 u L p 1 ( V ) p 1 λ M 6 ( μ , h 2 , ) k 2 p 2 p 2 v m 2 , p 2 k 2 p 2 v L p 2 ( V ) p 2 2 1 max { p 1 , p 2 } max { p 1 , p 2 } ( u , v ) max { p 1 , p 2 } λ M 5 μ k 1 p 1 p 1 h 1 , k 1 p 1 u m 1 , p 1 k 1 λ M 6 μ k 2 p 2 p 2 h 2 , k 2 p 2 v m 2 , p 2 k 2 2 1 max { p 1 , p 2 } max { p 1 , p 2 } ( u , v ) max { p 1 , p 2 } λ M 5 μ k 1 p 1 p 1 h 1 , k 1 p 1 + M 6 μ k 2 p 2 p 2 h 2 , k 2 p 2 ( u , v ) min { k 1 , k 2 } .

Let

ν 0 , λ = 2 1 max { p 1 , p 2 } λ max { p 1 , p 2 } M 5 μ k 1 p 1 p 1 h 1 , k 1 p 1 + M 6 μ k 2 p 2 p 2 h 2 , k 2 p 2 1 min { k 1 , k 2 } max { p 1 , p 2 } .

Then by (3.2), ν λ satisfies 0 < ν λ < min { 1 , ν 0 , λ } such that

I ¯ λ ( u , v ) 2 1 max { p 1 , p 2 } max { p 1 , p 2 } ν λ max { p 1 , p 2 } λ M 5 μ k 1 p 1 p 1 h 1 , k 1 p 1 + M 6 μ k 2 p 2 p 2 h 2 , k 2 p 2 ν λ min { k 1 , k 2 } η λ > 2 1 max { p 1 , p 2 } max { p 1 , p 2 } ν 0 , λ max { p 1 , p 2 } λ M 5 μ k 1 p 1 p 1 h 1 , k 1 p 1 + M 6 μ k 2 p 2 p 2 h 2 , k 2 p 2 ν 0 , λ min { k 1 , k 2 } = 0

for all ( u , v ) = ν λ .□

Lemma 3.3

Assume that ( H 5 ) holds. Then for each λ > max { Λ 1 , Λ 2 , Λ 3 , Λ 4 } , where Λ 1 , Λ 2 , Λ 3 , and Λ 4 are defined in (1.6), (1.7), (1.8), and (1.9), respectively, there exists ( u 0 , v 0 ) W m 1 , p 1 ( V ) \ { 0 } × W m 2 , p 2 ( V ) \ { 0 } with u 0 > 0 , v 0 > 0 , and ( u 0 , v 0 ) δ such that ( u 0 , v 0 ) > ν λ and I ¯ λ ( u 0 , v 0 ) < 0 .

Proof

Let ( u 0 , v 0 ) W m 1 , p 1 ( V ) \ { 0 } × W m 2 , p 2 ( V ) \ { 0 } with u 0 > 0 , v 0 > 0 for any x V and satisfies u 0 δ 2 and v 0 δ 2 . It is easy to see that ν 0 , λ < 1 for any λ > Λ 1 . We could take ν λ = 1 2 ν 0 , λ . By Remark 2.1, we have u 0 m 1 , p 1 > 1 3 ν λ for all λ > Λ 2 and v 0 m 2 , p 2 > 2 3 ν λ for all λ > Λ 3 , respectively. Then ( u 0 , v 0 ) = u 0 m 1 , p 1 + v 0 m 2 , p 2 > 1 3 ν λ + 2 3 ν λ = ν λ for all λ > max { Λ 2 , Λ 3 } . It follows from Remark 2.1, ( H 5 ) and Hölder’s inequality that

I ¯ λ ( u 0 , v 0 ) = 1 p 1 u 0 m 1 , p 1 p 1 + 1 p 2 v 0 m 2 , p 2 p 2 λ V F ¯ ( x , u 0 , v 0 ) d μ 1 p 1 max { 1 , h 1 } ( m 1 u 0 L p 1 ( V ) p 1 + u 0 L p 1 ( V ) p 1 ) + 1 p 2 max { 1 , h 2 } ( m 2 v 0 L p 2 ( V ) p 2 + v 0 L p 2 ( V ) p 2 ) λ M 1 x V μ ( x ) 1 q 1 p 1 u 0 L p 1 ( V ) q 1 + M 2 x V μ ( x ) 1 q 2 p 2 v 0 L p 2 ( V ) q 2 < 0

for all λ > Λ 4 .□

It follows from Lemmas 3.2, 3.3, and the fact I ¯ λ ( 0 , 0 ) = 0 that I ¯ λ has a mountain pass geometry, that is, setting

Γ { γ C ( [ 0 , 1 ] , W ) : γ ( 0 ) = ( 0 , 0 ) , γ ( 1 ) = ( u 0 , v 0 ) } .

Obviously, Γ . By Lemma 2.5, for the mountain pass level

c λ inf γ Γ max t [ 0 , 1 ] I ¯ λ ( γ ( t ) ) ,

there exists a ( C ) c λ -sequence { ( u n , v n ) } { ( u n , λ , v n , λ ) } of I ¯ λ in W , that is,

(3.3) I ¯ λ ( u n , v n ) c λ and ( 1 + ( u n , v n ) ) I ¯ λ ( u n , v n ) W * 0 , as n .

Moreover, Lemma 3.2 implies that c λ > 0 .

Lemma 3.4

Assume that ( H 3 ) holds. Then the ( C ) c λ -sequence { ( u n , v n ) } has a convergent subsequence for any given λ > 0 .

Proof

By (3.3), we have

( u n , v n ) I ¯ λ ( u n , v n ) W * 0 as n ,

which implies

(3.4) I ¯ λ ( u n , v n ) , 1 θ 1 u n , 1 θ 2 v n 1 min { θ 1 , θ 2 } I ¯ λ ( u n , v n ) W * ( u n , v n ) 0 as n .

Then by (3.3), (3.4), and ( H 3 ) , for n large enough and any λ > 0 , we have

(3.5) c λ + 1 I ¯ λ ( u n , v n ) I ¯ λ ( u n , v n ) , 1 θ 1 u n , 1 θ 2 v n = 1 p 1 1 θ 1 u n m 1 , p 1 p 1 + 1 p 2 1 θ 2 v n m 1 , p 2 p 2 + λ V 1 θ 1 u n F ¯ u ( x , u n , v n ) + 1 θ 2 v n F ¯ v ( x , u n , v n ) F ¯ ( x , u n , v n ) d μ 1 p 1 1 θ 1 u n m 1 , p 1 p 1 + 1 p 2 1 θ 2 v n m 1 , p 2 p 2 ,

which implies that { u n } and { v n } are bounded in W m 1 , p 1 ( V ) and W m 2 , p 2 ( V ) , respectively. As both W m 1 , p 1 ( V ) and W m 2 , p 2 ( V ) are precompact, up to a subsequence of { ( u n , v n ) } , still denoted by { ( u n , v n ) } , there exists ( u λ , v λ ) W such that u n u λ in W m 1 , p 1 ( V ) and v n v λ in W m 2 , p 2 ( V ) , respectively.□

Lemma 3.4 shows that ( u n , v n ) ( u λ , v λ ) in W , which together with (3.3) and the continuity of I ¯ λ and I ¯ λ imply that I ¯ λ ( u λ , v λ ) = c λ and I ¯ λ ( u λ , v λ ) = 0 . Moreover, by I ¯ λ ( 0 , 0 ) = 0 and c λ > 0 , we have ( u λ , v λ ) ( 0 , 0 ) . Thus, ( u λ , v λ ) is a nontrivial critical point of I ¯ λ with the critical value c λ . Next, we will show that ( u λ , v λ ) precisely is the nontrivial weak solution of system (1.4).

Lemma 3.5

Assume that ( H 3 ) and ( H 5 ) hold. Then there exist C 1 , * > 0 and C 2 , * > 0 independent of λ > 0 such that

u λ p 1 θ 1 max { C 1 , * , C 2 , * } ( θ 1 p 1 ) μ h 1 , 1 p 1 λ p 1 q 1 p 1 + λ p 2 q 2 p 2 1 p 1 , v λ p 2 θ 2 max { C 1 , * , C 2 , * } ( θ 2 p 2 ) μ h 2 , 1 p 2 λ p 1 q 1 p 1 + λ p 2 q 2 p 2 1 p 2 ,

where C 1 , * and C 2 , * are defined in (1.11), and (1.12), respectively.

Proof

Let s [ 0 , 1 ] . Then s ( u 0 , v 0 ) ( u 0 , v 0 ) δ , where ( u 0 , v 0 ) is given in Lemma 3.3. For all λ > 0 , by ( H 5 ) and Hölder’s inequality, we have

(3.6) I ¯ λ ( s u 0 , s v 0 ) = 1 p 1 u 0 m 1 , p 1 p 1 s p 1 + 1 p 2 v 0 m 2 , p 2 p 2 s p 2 λ V F ¯ ( x , s u 0 , s v 0 ) d μ 1 p 1 u 0 m 1 , p 1 p 1 s p 1 + 1 p 2 v 0 m 2 , p 2 p 2 s p 2 λ M 1 s q 1 V u 0 q 1 d μ λ M 2 s q 2 V v 0 q 2 d μ 1 p 1 u 0 m 1 , p 1 p 1 s p 1 λ M 1 x V μ ( x ) 1 q 1 p 1 u 0 L p 1 ( V ) q 1 s q 1 + 1 p 2 v 0 m 2 , p 2 p 2 s p 2 λ M 2 x V μ ( x ) 1 q 2 p 2 v 0 L p 2 ( V ) q 2 s q 2 .

Define g i : [ 0 , + ) R , i = 1 , 2, by

g 1 ( s ) = 1 p 1 u 0 m 1 , p 1 p 1 s p 1 λ M 1 x V μ ( x ) 1 q 1 p 1 u 0 L p 1 ( V ) q 1 s q 1 , g 2 ( s ) = 1 p 2 v 0 m 2 , p 2 p 2 s p 2 λ M 2 x V μ ( x ) 1 q 2 p 2 v 0 L p 2 ( V ) q 2 s q 2 .

For any λ > 0 , let

g 1 ( s ) = s p 1 1 u 0 m 1 , p 1 p 1 λ q 1 M 1 x V μ ( x ) 1 q 1 p 1 u 0 L p 1 ( V ) q 1 s q 1 p 1 = 0 .

Then we have s 1 λ = x V μ ( x ) 1 p 1 u 0 m 1 , p 1 p 1 λ q 1 M 1 u 0 L p 1 ( V ) q 1 1 q 1 p 1 > 0 . It follows from Remark 2.1 that

(3.7) max s 0 g 1 ( s ) = g 1 ( s 1 λ ) = ( q 1 p 1 ) x V μ ( x ) p 1 u 0 m 1 , p 1 u 0 L p 1 ( V ) p 1 q 1 q 1 p 1 ( q 1 q 1 M 1 p 1 ) 1 p 1 q 1 λ p 1 q 1 p 1

(3.7) ( q 1 p 1 ) x V μ ( x ) p 1 ( m 1 u 0 L p 1 ( V ) p 1 + u 0 L p 1 ( V ) p 1 ) 1 p 1 u 0 L p 1 ( V ) p 1 q 1 q 1 p 1 × ( max { 1 , h 1 } ) q 1 q 1 q 1 M 1 p 1 1 q 1 p 1 λ p 1 q 1 p 1 = C 1 , * λ p 1 q 1 p 1 .

Similarly, we have

(3.8) max s 0 g 2 ( s ) = g 2 ( s 2 λ ) C 2 , * λ p 2 q 2 p 2 ,

where s 2 λ = x V μ ( x ) 1 p 2 v 0 m 2 , p 2 p 2 λ q 2 M 2 v 0 L p 2 ( V ) q 2 1 q 2 p 2 > 0 . By the definition of c λ , (3.6), (3.7), and (3.8), we have

(3.9) c λ max s [ 0 , 1 ] I ¯ λ ( s u 0 , s v 0 ) max s 0 g 1 ( s ) + max s 0 g 2 ( s ) max { C 1 , * , C 2 , * } λ p 1 q 1 p 1 + λ p 2 q 2 p 2 .

Note that I ¯ λ ( u λ , v λ ) , ( 1 θ 1 u λ , 1 θ 2 v λ ) = 0 . Similar to the argument in (3.5), we have

u λ m 1 , p 1 p 1 θ 1 θ 1 p 1 1 p 1 c λ 1 p 1 , v λ m 2 , p 2 p 2 θ 2 θ 2 p 2 1 p 2 c λ 1 p 2 ,

which combining with (3.9) connote that

(3.10) u λ m 1 , p 1 p 1 θ 1 max { C 1 , * , C 2 , * } θ 1 p 1 1 p 1 λ p 1 q 1 p 1 + λ p 2 q 2 p 2 1 p 1

and

(3.11) v λ m 2 , p 2 p 2 θ 2 max { C 1 , * , C 2 , * } θ 2 p 2 1 p 2 λ p 1 q 1 p 1 + λ p 2 q 2 p 2 1 p 2 .

By Lemma 2.2, we further obtain the following results:

(3.12) u λ p 1 θ 1 max { C 1 , * , C 2 , * } ( θ 1 p 1 ) μ h 1 , 1 p 1 λ p 1 q 1 p 1 + λ p 2 q 2 p 2 1 p 1

and

(3.13) v λ p 2 θ 2 max { C 1 , * , C 2 , * } ( θ 2 p 2 ) μ h 2 , 1 p 2 λ p 1 q 1 p 1 + λ p 2 q 2 p 2 1 p 2 .

The proof is completed.□

Proof of Theorem 1.1

It follows from the fact q i > p i > 1 , i = 1 , 2 and Lemma 2.4 that

λ p 1 q 1 p 1 + λ p 2 q 2 p 2 2 1 + λ max p 1 q 1 p 1 , p 2 q 2 p 2 ,

which together with Lemma 3.5 implies that ( u λ , v λ ) u λ + v λ δ 4 + δ 4 = δ 2 for each λ > Λ 5 , where Λ 5 is defined in (1.10). Therefore, ( u λ , v λ ) W is a nontrivial weak solution of system (1.4). Furthermore, (3.10)–(3.13) imply that

( u λ , v λ ) p 1 θ 1 max { C 1 , * , C 2 , * } θ 1 p 1 1 p 1 λ p 1 q 1 p 1 + λ p 2 q 2 p 2 1 p 1 + p 2 θ 2 max { C 1 , * , C 2 , * } θ 2 p 2 1 p 2 λ p 1 q 1 p 1 + λ p 2 q 2 p 2 1 p 2

and

( u λ , v λ ) p 1 θ 1 max { C 1 , * , C 2 , * } ( θ 1 p 1 ) μ h 1 , 1 p 1 λ p 1 q 1 p 1 + λ p 2 q 2 p 2 1 p 1 + p 2 θ 2 max { C 1 , * , C 2 , * } ( θ 2 p 2 ) μ h 2 , 1 p 2 λ p 1 q 1 p 1 + λ p 2 q 2 p 2 1 p 2 .

Thus, we have lim λ ( u λ , v λ ) = 0 = lim λ ( u λ , v λ ) .

4 Proofs for the sublinear case

Define ρ ( t , s ) C 1 ( R 2 , [ 0 , 1 ] ) as a cut-off function satisfying

ρ ( t , s ) = 1 , if ( t , s ) δ 2 , 0 , if ( t , s ) > δ .

Define F ˜ : V × R × R R by

F ˜ ( x , t , s ) = ρ ( t , s ) F ( x , t , s ) + ( 1 ρ ( t , s ) ) ( K 1 t q 1 + K 2 s q 2 ) .

By ( H 0 ) , ( R 2 ) ( R 4 ) , and the definition of ρ ( t , s ) , we could obtain the following lemma:

Lemma 4.1

Assume that ( H 0 ) , ( R 2 ) ( R 4 ) hold. Then

  1. F ˜ ( x , t , s ) is continuously differentiable in R × R for all x V ;

  2. there exist K 7 > 0 and K 8 > 0 such that

    F ˜ t ( x , t , s ) K 7 ( t q 1 1 + t k 1 1 ) + K 8 s k 2 ( k 1 1 ) k 1 , F ˜ s ( x , t , s ) K 7 t k 1 ( k 2 1 ) k 2 + K 8 ( s q 2 1 + s k 2 1 ) ,

    for all x V and ( t , s ) R 2 ;

  3. F ˜ ( x , t , s ) = F ˜ ( x , t , s ) for all x V and ( t , s ) R 2 ;

  4. K 1 t q 1 + K 2 s q 2 F ˜ ( x , t , s ) max { K 1 , K 5 } ( t q 1 + t k 1 ) + max { K 2 , K 6 } ( s q 2 + s k 2 )

    for all x V and ( t , s ) R 2 .

Consider the modified system of (1.4) given by

(4.1) £ m 1 , p 1 u + h 1 ( x ) u p 1 2 u = λ F ˜ u ( x , u , v ) , x V , £ m 2 , p 2 v + h 2 ( x ) v p 2 2 v = λ F ˜ v ( x , u , v ) , x V .

Define the corresponding functional I ˜ λ : W R by

I ˜ λ ( u , v ) 1 p 1 V ( m 1 u p 1 + h 1 ( x ) u p 1 ) d μ + 1 p 2 V ( m 2 v p 2 + h 2 ( x ) v p 2 ) d μ λ V F ˜ ( x , u , v ) d μ

for all ( u , v ) W . By ( R 0 ) ( R 4 ) and the continuous embeddings

W m i , p i ( V ) L q i ( V ) , W m i , p i ( V ) L k i ( V ) , i = 1 , 2 ,

standard arguments show that I ˜ λ is well defined, even and of class C 1 on W , and

I ˜ λ ( u , v ) , ( ϕ 1 , ϕ 2 ) = V ( £ m 1 , p 1 u ϕ 1 + h 1 ( x ) u p 1 2 u ϕ 1 ) d μ + V ( £ m 2 , p 2 v ϕ 2 + h 2 ( x ) v p 2 2 v ϕ 2 ) d μ λ V F ˜ u ( x , u , v ) ϕ 1 d μ λ V F ˜ v ( x , u , v ) ϕ 2 d μ

for all ( u , v ) , ( ϕ 1 , ϕ 2 ) W [40]. Hence,

I ˜ λ ( u , v ) , ( u , v ) = u m 1 , p 1 p 1 + v m 2 , p 2 p 2 λ V F ˜ u ( x , u , v ) u d μ λ V F ˜ v ( x , u , v ) v d μ

for all ( u , v ) W . Note that the critical points of I ˜ λ with L -norm less than or equal to δ 2 are also critical points of I λ . Then the weak solutions of system (4.1) with L -norm less than or equal to δ 2 are also weak solutions of problem (1.4).

Proof of Theorem 1.3

Obviously, I ˜ λ C 1 ( W , R ) is even and I ˜ λ ( 0 , 0 ) = 0 . For any fixed λ > 0 , using ( R 4 ) , we obtain

I ˜ λ ( u , v ) 1 p 1 u m 1 , p 1 p 1 λ max { K 1 , K 5 } V ( u q 1 + u k 1 ) d μ + 1 p 2 v m 2 , p 2 p 2 λ max { K 2 , K 6 } V ( v q 2 + v k 2 ) d μ ,

which estimate by Lemma 2.3 leads to

I ˜ λ ( u , v ) 1 p 1 u m 1 , p 1 p 1 λ max { K 1 , K 5 } x V μ ( x ) 1 μ q 1 p 1 h 1 , q 1 p 1 u m 1 , p 1 q 1 + 1 μ k 1 p 1 h 1 , k 1 p 1 u m 1 , p 1 k 1 + 1 p 2 v m 2 , p 2 p 2 λ max { K 2 , K 6 } x V μ ( x ) 1 μ q 2 p 2 h 2 , q 2 p 2 v m 2 , p 2 q 2 + 1 μ k 2 p 2 h 2 , k 2 p 2 v m 2 , p 2 k 2 ,

which together with the fact p i > q i > k i > 1 ( i = 1 , 2 ) implies that I ˜ λ ( u , v ) + as ( u , v ) . So, I ˜ λ is coercive and bounded form below on W . Suppose that { ( u n , v n ) } is a Palais-Smale sequence of I ˜ λ on W , that is,

{ I ˜ λ ( u n , v n ) } is bounded , I ˜ λ ( u n , v n ) 0 as n .

Then the coercivity of I ˜ λ implies that { ( u n , v n ) } is bounded on W . Due to both W m 1 , p 1 ( V ) and W m 2 , p 2 ( V ) are pre-compact, up to a subsequence of { ( u n , v n ) } , still denoted by { ( u n , v n ) } , there exists ( u ˜ λ , v ˜ λ ) W such that u n u ˜ λ in W m 1 , p 1 ( V ) and v n v ˜ λ in W m 2 , p 2 ( V ) , respectively. Hence, functional I ˜ λ satisfies the Palais-Smale condition for all λ > 0 . Let Z k be a k -dimensional subspace of W for any k N . Then all norms are equivalent in Z k . Hence, there exist positive constants c 1 and c 2 such that

(4.2) u L q 1 ( V ) q 1 c 1 u m 1 , p 1 q 1 , v L q 2 ( V ) q 2 c 2 v m 2 , p 2 q 2

for all ( u , v ) Z k . For any given 0 < ρ k < min { 1 , ρ λ } ,

ρ λ = p 1 p 2 p 1 + p 2 λ min { K 1 c 1 , K 2 c 2 } 2 1 max { q 1 , q 2 } 1 min { p 1 , p 2 } max { q 1 , q 2 } ,

define

S ρ k = { ( u , v ) W ( u , v ) = ρ k } .

By ( R 4 ) , (4.2), and the fact min { p 1 , p 2 } > max { q 1 , q 2 } , we have

I ˜ λ ( u , v ) = 1 p 1 u m 1 , p 1 p 1 + 1 p 2 v m 2 , p 2 p 2 λ V F ˜ ( x , u , v ) d μ p 1 + p 2 p 1 p 2 ( u , v ) min { p 1 , p 2 } λ K 1 V u q 1 d μ λ K 2 V v q 2 d μ

p 1 + p 2 p 1 p 2 ( u , v ) min { p 1 , p 2 } λ K 1 c 1 u m 1 , p 1 q 1 λ K 2 c 2 v m 2 , p 2 q 2 p 1 + p 2 p 1 p 2 ( u , v ) min { p 1 , p 2 } λ K 1 c 1 u m 1 , p 1 max { q 1 , q 2 } λ K 2 c 2 v m 2 , p 2 max { q 1 , q 2 } p 1 + p 2 p 1 p 2 ( u , v ) min { p 1 , p 2 } λ min { K 1 c 1 , K 2 c 2 } ( u m 1 , p 1 max { q 1 , q 2 } + v m 2 , p 2 max { q 1 , q 2 } ) p 1 + p 2 p 1 p 2 ( u , v ) min { p 1 , p 2 } λ min { K 1 c 1 , K 2 c 2 } 2 1 max { q 1 , q 2 } ( u , v ) max { q 1 , q 2 } < 0

for any ( u , v ) Z k S ρ k and λ > 0 . So sup Z k S ρ k I ˜ λ < 0 . Hence, Lemma 2.6 and Remark 2.7 show that system (4.1) has infinitely many nonzero solutions { ( u k λ , v k λ ) } such that ( u k λ , v k λ ) 0 as k . By Lemma 2.2, we further obtain

( u k λ , v k λ ) u k λ + v k λ max 1 μ 1 p 1 h 1 , 1 p 1 , 1 μ 1 p 2 h 2 , 1 p 2 ( u k λ , v k λ ) 0 as k .

So there exists a sufficiently large integer k 0 > 0 such that ( u k λ , v k λ ) δ 2 for all k k 0 , which implies that { ( u k λ , v k λ ) } k 0 is a sequence of weak solutions of the original system (1.4) for each fixed λ > 0 .□

5 Examples

In this section, we present two examples that satisfy the conditions of Theorems 1.1 and 1.3, respectively.

Example 5.1

Let G = ( V , E ) is a finite graph, specifically,

V = { x 1 , x 2 , x 3 , x 4 , x 5 , x 6 , x 7 } , E = { { x 1 , x 2 } , { x 1 , x 3 } , { x 1 , x 4 } , { x 1 , x 5 } , { x 2 , x 3 } , { x 2 , x 6 } , { x 3 , x 4 } , { x 4 , x 7 } , { x 5 , x 6 } , { x 5 , x 7 } } , μ ( x 1 ) = 2 , μ ( x 2 ) = 1 , μ ( x 3 ) = μ ( x 4 ) = 3 , μ ( x 5 ) = μ ( x 6 ) = 5 , μ ( x 7 ) = 6 and deg ( x 1 ) = 6 .

Then V 1 d μ = Σ x V μ ( x ) = 25 . Let A = { x V x x 1 } and A = 4 , where A is the number of elements in the set A . Let

e 1 ( x ) = e 2 ( x ) = 1 , if x = x 1 , 0 , if x x 1 .

Choose

(5.1) u 0 = δ μ 1 2 h 1 , 1 2 2 17 ( max { 1 , h 1 } ) 1 2 e 1 and v 0 = δ μ 1 2 h 2 , 1 2 2 17 ( max { 1 , h 2 } ) 1 2 e 2 .

Let δ = 1 , m 1 = m 2 = 1 , p 1 = p 2 = 2 , and h 1 ( x ) = h 2 ( x ) = 1 for all x V . Consider the following system:

(5.2) Δ u + u = λ F u ( x , u , v ) , x V , Δ v + v = λ F v ( x , u , v ) , x V ,

where

F ( x , t , s ) = σ ( t , s ) ( t 6 + s 6 ) + ( 1 σ ( t , s ) ) ( t 4 + s 4 )

for all ( x , t , s ) V × R × R with σ ( t , s ) defined by

σ ( t , s ) = 1 , if ( t , s ) 1 , sin π ( t 2 + s 2 16 ) 2 450 , if 1 < ( t , s ) 4 , 0 , if ( t , s ) > 4 .

So,

F ( x , t , s ) = t 6 + s 6 , if ( t , s ) 1 , ( t 6 + s 6 ) sin π ( t 2 + s 2 16 ) 2 450 + 1 sin π ( t 2 + s 2 16 ) 2 450 ( t 4 + s 4 ) , if 1 < ( t , s ) 4 , t 4 + s 4 , if ( t , s ) > 4 .

By Theorem 1.1, we can obtain that system (5.2) has at least a nontrivial weak solution ( u λ , v λ ) for each λ > Λ 4 89523333.3 and lim λ ( u λ , v λ ) = 0 = lim λ ( u λ , v λ ) .

In fact, we can verify that F satisfies the conditions in Theorem 1.1. Let

A ( t , s ) 6 t 4 t sin π ( t 2 + s 2 16 ) 2 450 + 4 1 sin π ( t 2 + s 2 16 ) 2 450 b ( x ) t 2 t + ( t 6 + s 6 ) 2 π t ( t 2 + s 2 16 ) 225 cos π ( t 2 + s 2 16 ) 2 450 ( t 4 + s 4 ) 2 π t ( t 2 + s 2 16 ) 225 cos π ( t 2 + s 2 16 ) 2 450 ,

and

B ( t , s ) 6 s 4 s sin π ( t 2 + s 2 16 ) 2 450 + 4 1 sin π ( t 2 + s 2 16 ) 2 450 s 2 s + ( t 6 + s 6 ) 2 π s ( t 2 + s 2 16 ) 225 cos π ( t 2 + s 2 16 ) 2 450 ( t 4 + s 4 ) 2 π s ( t 2 + s 2 16 ) 225 cos π ( t 2 + s 2 16 ) 2 450 .

It is easy to see that F satisfies ( H 0 ) and

F t ( x , t , s ) = 6 t 4 t , if ( t , s ) 1 , A ( t , s ) , if 1 < ( t , s ) 4 , 4 t 2 t , if ( t , s ) > 4 ,

F s ( x , t , s ) = 6 s 4 s , if ( t , s ) 1 , B ( t , s ) , if 1 < ( t , s ) 4 , 4 s 2 s , if ( t , s ) > 4 .

Hence, we obtain

F ( x , t , s ) = t 6 + s 6 t 7 + s 7 , for all x V and ( t , s ) 1 .

Then ( H 1 ) holds with q 1 = q 2 = 7 > 2 = p 1 = p 2 , M 1 = M 2 = 1 . We also have

F t ( x , t , s ) = 6 t 5 6 ( t 4 + s 4 ) , for all x V and ( t , s ) 1 .

Similarly,

F s ( x , t , s ) 6 ( t 4 + s 4 ) , for all x V and ( t , s ) 1 .

Then ( H 2 ) holds with k 1 = k 2 = 5 ( 2, 7 ) and M 3 = M 4 = 6 . In particular, taking β 1 = β 2 = 3 > 2 = p 1 = p 2 , we have

F ( x , t , s ) = t 6 + s 6 2 ( t 6 + s 6 ) = 1 β 1 t F t ( x , t , s ) + 1 β 2 s F s ( x , t , s )

for all x R N and ( t , s ) 1 . Thus, assumption ( H 3 ) is satisfied.

Next, we complete the value of λ by the formulas in Theorem 1.1. It follows that

(5.3) e 1 L 2 ( V ) 2 = x V e 1 2 ( x ) μ ( x ) = x V 1 2 μ ( x ) y x ω x y ( e 1 ( y ) e 1 ( x ) ) 2 μ ( x ) = 1 2 μ ( x 1 ) y x 1 ω x 1 y μ ( x 1 ) + x x 1 1 2 μ ( x ) x 1 x ω x x 1 μ ( x ) = 1 2 deg ( x 1 ) ( 1 + A ) = 15 = e 2 L 2 ( V ) 2 .

Similarly, we have

(5.4) e 1 L 2 ( V ) 2 = e 2 L 2 ( V ) 2 = μ ( x 1 ) = 2 .

By Lemma 2.2, Remark 2.1, (5.3), (5.4), and (5.1), we have

0 < u 0 δ 2 and 0 < v 0 δ 2 .

Moreover,

u 0 L 2 ( V ) 2 = 15 δ 2 μ h 1 , 68 max { 1 , h 1 } , v 0 L 2 ( V ) 2 = 15 δ 2 μ h 2 , 68 max { 1 , h 2 } , u 0 L 2 ( V ) 2 = δ 2 μ h 1 , 34 max { 1 , h 1 } , v 0 L 2 ( V ) 2 = δ 2 μ h 2 , 34 max { 1 , h 2 } .

Then by θ 1 = θ 2 = 3 , M 5 = 12 5 , M 6 = 6 , h 1 , = h 2 , = 1 = h 1 = h 2 , μ = min x V μ ( x ) = 1 , (1.11) and (1.12), we have

C 1 , * = C 2 , * = 125 2 17 14 7 5 ,

and by (1.6)–(1.10),

Λ 1 = 5 168 , Λ 2 = 5 168 ( 6 ) 3 ( 34 ) 3 2 , Λ 3 = 5 168 ( 3 ) 3 ( 34 ) 3 2 , Λ 4 = 17 136 ( 25 ) 5 2 ( 34 ) 7 2 , Λ 5 = ( 2 ) 9 ( 3 ) 5 2 ( 5 ) 15 2 ( 17 ) 7 2 ( 7 ) 7 5 3 ( 5 ) 3 ( 2 ) 18 5 ( 17 ) 7 5 5 2 .

Compared Λ 1 , Λ 2 , Λ 3 , Λ 4 , and Λ 5 , it is easy to see λ = Λ 4 89523333.3 .

Remark 5.2

Through the conclusion of Theorem 1.1 and the calculations for the parameter λ in Example 5.1, it is easy to see the following interesting phenomenon: the specific lower bound of the parameter on a finite graph is related to the structure of the graph, such as the degree and the measure of any point in V . However, in the Euclidean setting, in general, the specific lower bound is only related to the measure of domain [17]. The fundamental reason for this distinction lies in the difference between the definitions of integrals on the graph and in Euclidean space.

Example 5.3

Let G = ( V , E ) is a finite graph, δ = 1 , m 1 = m 2 = 1 , p 1 = 2 , p 2 = 3 , and h 1 ( x ) = h 2 ( x ) = 1 for all x V . Consider the following system:

(5.5) Δ u + u = λ F u ( x , u , v ) , x V , Δ 3 v + v v = λ F v ( x , u , v ) , x V ,

where

F ( x , t , s ) = 3 4 ( t 4 3 + s 4 3 )

for all ( x , t , s ) V × R × R . By Theorem 1.2, we can obtain that system (5.5) has a sequence of weak solutions { ( u k λ , v k λ ) } with ( u k λ , v k λ ) 0 as k for every λ > 0 .

In fact, we can verify that F satisfies the conditions in Theorem 1.3. It is easy to see that ( H 0 ) , ( H 4 ) , and ( R 3 ) hold. We also have ( R 1 ) holds with q 1 = q 2 = 5 3 ( 1 , 2 ) and K 1 = K 2 = 3 4 . It follows that

F t ( x , t , s ) = t 1 3 2 ( t 1 4 + s 1 4 ) , for all x V and ( t , s ) 1 .

Similarly,

F s ( x , t , s ) 2 ( t 1 4 + s 1 4 ) , for all x V and ( t , s ) 1 .

Then ( R 2 ) holds with k 1 = k 2 = 5 4 ( 1 , 5 3 ) and K 3 = K 4 = 2 .

Acknowledgments

The authors sincerely thank the reviewers for their valuable comments.

  1. Funding information: This project was supported by Yunnan Fundamental Research Projects (grant No: 202301AT070465) and Xingdian Talent Support Program for Young Talents of Yunnan Province.

  2. Author contributions: Wanting Qi and Xingyong Zhang contributed to the main manuscript equally.

  3. Conflict of interest: The authors declare that they have no conflict of interest.

  4. Ethical approval: Not applicable.

  5. Data availability statement: No data were used in this study.

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Received: 2024-09-07
Revised: 2025-02-22
Accepted: 2025-06-17
Published Online: 2025-07-31

© 2025 the author(s), published by De Gruyter

This work is licensed under the Creative Commons Attribution 4.0 International License.

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  129. Ground state solutions to singularly perturbed Chern-Simons-Schrödinger systems with a neutral scalar field
  130. Weak solutions to an asymptotic equation of the variational sine-Gordon equation
  131. Multiplicity of positive solutions for a concave-convex fractional elliptic system with critical growth
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